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Using spectral shape and predictor fluence to evaluate temporal dependence of exposures from solar particle events

机译:使用光谱形状和预测因子密度来评估太阳粒子事件暴露的时间依赖性

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Real-time estimation of exposure levels has been considered in NASA's operational strategies and structural capability for the protection of astronauts from exposure to large solar particle events (SPEs). The temporal profile of organ dose rates is also important for the analysis of dose-rate-dependent biological responses and the optimization of radiation shielding and future mission planning. A realistic temporal estimation of exposure profiles relies on (1) the complete energy spectrum of SPE that defines the boundary condition for radiation transport simulation, (2) the radiation transport simulation with detailed shielding and body geometry models that determines particle transmission at each critical body organ, and (3) the assessment of organ dosimetric quantities and biological risks by applying the corresponding response models. This paper introduces a process of rapidly estimating temporal exposures to SPEs by implementing the distributions of the organ doses and the spectral-shape characterization of the major SPEs. Simultaneously, the unconditional probability exceeding the NASA 30 day limit of a blood-forming organ dose is estimated by taking into account the variability of detailed spectra of SPEs for a given predictor fluence. These temporal evaluations of SPEs can be applied to the development of real-time guidance and protection system on improving mitigation of adverse effects during space missions.
机译:NASA的操作策略和结构能力已经考虑到了暴露水平的实时估计,以保护宇航员免受大太阳粒子事件(SPE)的暴露。器官剂量率的时间曲线对于分析剂量率依赖性的生物反应以及优化辐射屏蔽和未来任务规划也很重要。实际的时间估算暴露曲线依赖于(1)SPE的完整能谱,该谱定义了辐射传输模拟的边界条件,(2)带有详细屏蔽和物体几何模型的辐射传输模拟,确定了每个关键物体的粒子透射率(3)通过使用相应的响应模型评估器官剂量和生物学风险。本文介绍了通过实现器官剂量的分布和主要SPE的光谱形状表征来快速估算SPE的时间暴露的过程。同时,通过考虑给定预测能量密度下SPE详细光谱的可变性,可以估算出无条件概率超过NASA 30天限度的造血器官剂量。这些SPE的时间评估可用于开发实时制导和保护系统,以改善空间飞行任务期间的不良影响。

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